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Phys."],"abstract":"<jats:title>\n                    A\n                    <jats:sc>bstract<\/jats:sc>\n                  <\/jats:title>\n                  <jats:p>\n                    The modifications imprinted on jets due to their interaction with Quark Gluon Plasma (QGP) are assessed by comparing samples of jets produced in nucleus-nucleus collisions and proton-proton collisions. The standard procedure ignores the effect of bin migration by comparing specific observables for jet populations at the same reconstructed jet transverse momentum (\n                    <jats:italic>p<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>T<\/jats:italic>\n                    <\/jats:sub>\n                    ). Since jet\n                    <jats:italic>p<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>T<\/jats:italic>\n                    <\/jats:sub>\n                    is itself modified by interaction with QGP, all such comparisons confound QGP induced modifications with changes that are simply a consequence of comparing jets that started out differently. The quantile matching procedure introduced by Brewer et al. directly estimates average fractional jet energy loss (\n                    <jats:italic>Q<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>AA<\/jats:italic>\n                    <\/jats:sub>\n                    ) and can thus mitigate this\n                    <jats:italic>p<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>T<\/jats:italic>\n                    <\/jats:sub>\n                    migration effect. In this work, we validate the procedure in more realistic scenarios that include medium response. We study the evolution of\n                    <jats:italic>Q<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>AA<\/jats:italic>\n                    <\/jats:sub>\n                    with jet radius, its sensitivity to minimum particle\n                    <jats:italic>p<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>T<\/jats:italic>\n                    <\/jats:sub>\n                    and medium response as implemented in two different models for jet evolution in heavy-ion collisions. Further, we use this procedure to establish that the difference between inclusive jet and\n                    <jats:italic>\u03b3<\/jats:italic>\n                    +jet nuclear modification factors (\n                    <jats:italic>R<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>AA<\/jats:italic>\n                    <\/jats:sub>\n                    ) is dominated by differences in the spectral shape, leaving the colour charge of the jet initiating parton with a lesser role to play. Additionally, we compare\n                    <jats:italic>Q<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>AA<\/jats:italic>\n                    <\/jats:sub>\n                    to an experimentally proposed proxy for fractional jet energy loss,\n                    <jats:italic>S<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>loss<\/jats:italic>\n                    <\/jats:sub>\n                    , showing that both quantities are similar, although the former provides a more clear physical interpretation. Finally, we show the size of the\n                    <jats:italic>p<\/jats:italic>\n                    <jats:sub>\n                      <jats:italic>T<\/jats:italic>\n                    <\/jats:sub>\n                    migration correction for four different substructure observables and how to reliably use the quantile procedure experimentally to improve existing measurements.\n                  <\/jats:p>","DOI":"10.1007\/jhep01(2025)164","type":"journal-article","created":{"date-parts":[[2025,2,1]],"date-time":"2025-02-01T11:54:13Z","timestamp":1738410853000},"update-policy":"https:\/\/doi.org\/10.1007\/springer_crossmark_policy","source":"Crossref","is-referenced-by-count":4,"title":["Towards an unbiased jet energy loss measurement"],"prefix":"10.1007","volume":"2025","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-3500-9681","authenticated-orcid":false,"given":"Liliana","family":"Apolin\u00e1rio","sequence":"first","affiliation":[{"id":[{"id":"https:\/\/ror.org\/01hys1667","id-type":"ROR","asserted-by":"publisher"}],"name":"LIP"},{"id":[{"id":"https:\/\/ror.org\/01c27hj86","id-type":"ROR","asserted-by":"publisher"}],"name":"Instituto Superior T\u00e9cnico, Universidade de Lisboa"}]},{"ORCID":"https:\/\/orcid.org\/0009-0003-0353-3515","authenticated-orcid":false,"given":"L\u00e9nea","family":"Lu\u00eds","sequence":"additional","affiliation":[{"id":[{"id":"https:\/\/ror.org\/01hys1667","id-type":"ROR","asserted-by":"publisher"}],"name":"LIP"},{"id":[{"id":"https:\/\/ror.org\/01c27hj86","id-type":"ROR","asserted-by":"publisher"}],"name":"Instituto Superior T\u00e9cnico, Universidade de Lisboa"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-8154-3688","authenticated-orcid":false,"given":"Jos\u00e9 Guilherme","family":"Milhano","sequence":"additional","affiliation":[{"id":[{"id":"https:\/\/ror.org\/01hys1667","id-type":"ROR","asserted-by":"publisher"}],"name":"LIP"},{"id":[{"id":"https:\/\/ror.org\/01c27hj86","id-type":"ROR","asserted-by":"publisher"}],"name":"Instituto Superior T\u00e9cnico, Universidade de Lisboa"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-1978-408X","authenticated-orcid":false,"given":"Jo\u00e3o M.","family":"Silva","sequence":"additional","affiliation":[{"id":[{"id":"https:\/\/ror.org\/01hys1667","id-type":"ROR","asserted-by":"publisher"}],"name":"LIP"},{"id":[{"id":"https:\/\/ror.org\/01c27hj86","id-type":"ROR","asserted-by":"publisher"}],"name":"Instituto Superior T\u00e9cnico, Universidade de Lisboa"}]}],"member":"297","published-online":{"date-parts":[[2025,1,29]]},"reference":[{"key":"25403_CR1","unstructured":"PHENIX collaboration, Suppression of hadrons with large transverse momentum in central Au+Au collisions at $$ \\sqrt{s_{NN}} $$ = 130 GeV, Phys. 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